We discuss a new technology that promises large, inexpensive mirrors. We ar
gue that it should be possible to tilt a rotating viscous liquid by perhaps
as much as a few tens of degrees. The tilted liquid parabolic surface is u
sed as the support for a thin reflecting metallic film. It may also be poss
ible to use it to support an ultrathin glass mirror. We demonstrate two cri
tical steps: that a viscous liquid mirror can be tilted and that an optical
-quality metallic film can be deposited on a liquid. The advent of astronom
ically useful tilted floating-mirror telescopes is contingent on the develo
pment of high-viscosity, high-reflectivity liquids. It is a good omen that
we already have identified two classes of such liquids; however, there rema
in technical challenges to overcome before such liquids can be used in viab
le telescopes.